arXiv · astro-ph/0404483
Pulsar kicks and dark matter from a sterile neutrino
Abstract
The observed velocities of radio pulsars, which range in the hundreds kilometers per second, and many of which exceed 1000 km/s, are not explained by the standard physics of the supernova explosion. However, if a sterile neutrino with mass in the 1-20 keV range exists, it would be emitted asymmetrically from a cooling neutron star, which could give it a sufficient recoil to explain the pulsar motions. The same particle can be the cosmological dark mater. Future observations of X-ray telescopes and gravitational wave detectors can confirm or rule out this explanation.
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Alexander Kusenko. 2004-04-26. Pulsar kicks and dark matter from a sterile neutrino. https://doi.org/10.1142/s0217751x0502402x
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